All Tables

Table 1: Evolutionary tracks and stellar libraries used in the SSP libraries.
Table 2: Wavelength ranges that were not used for the spectral fit.
Table 3: Possible values of the population parameters.
Table A.1: H $_{\beta }$ equivalent widths, ${\Delta \log Q\rm (H^0)}$ parameters, mass ratios (relative to the total stellar mass), and ages of the individual sub-populations for each spectrum.